This conference thesis summarizes my presentation at Tartu Tuorla Cosmology meeting based on a collaborative work with E.Nardi and C.Smarra \cite{Muursepp:2024mbb}. It is well known that a pseudo-Nambu Goldstone boson (pNGB) coupled to a confining gauge group obtains a non-zero contribution to its mass through instanton effects. At non-zero temperature, this manifests in temperature-dependent mass $m^{2}(T) \propto T^{-n}$. If these particles come to dominate the energy density of the Universe in the non-relativistic regime they would accelerate the expansion of the Universe for $n>2$, thus providing a dark energy (DE) component. In this work, we outline a scenario in which a pNGB $\phi_{b}$ presently undergoing confinement could realize such a scenario. Using energetic considerations we find that $\phi_{b}$ alone is not enough to produce the experimentally observed amount of DE. However, coupling $\phi_{b}$ to the QCD axion $\phi_a$ allows the transfer of energy from the QCD axion to the pNGB via non-adiabatic level-crossing thus reproducing the observed amount of dark matter (DM) and DE.
Comment: Presentation of collaborative work with Enrico Nardi and Clemente Smarra, based on 2405.00090 [hep-ph] at Tartu-Tuorla cosmology conference, Borderless Universe on 08.05.2024